The Bohr model of hydrogen
Statement
For a one-electron atom or ion with nuclear charge \(+Ze\) (hydrogen has \(Z=1\)), postulate that the electron moves in a circular orbit under the Coulomb attraction of the nucleus, and that its orbital angular momentum is quantised in integer multiples of \(\hbar\): \(L=n\hbar\), \(n=1,2,3,\dots\). Then only discrete orbital radii and energies are allowed, with the electron's total energy given by \(E_n=-\dfrac{Z^2}{n^2}\cdot\dfrac{m_ee^4}{8\varepsilon_0^2h^2}=-\dfrac{13.6\,Z^2}{n^2}\text{ eV}\), and orbital radius \(r_n=\dfrac{n^2}{Z}a_0\), where \(a_0=\dfrac{\varepsilon_0h^2}{\pi m_ee^2}\approx0.529\,\text{Å}\) is the Bohr radius.
Why it matters
The Bohr model is the first physical picture that explains why hydrogen emits light only at specific, discrete wavelengths rather than a continuous spectrum — the empirical Rydberg formula, known since 1888 but unexplained, falls directly out of this result as the energy difference between two allowed levels. It is the bridge between the classical planetary picture of the atom (Rutherford, 1911) and full quantum mechanics: it keeps a classical orbit but imposes one quantum rule on top of it, and that single rule is enough to derive the entire hydrogen spectrum from first principles for the first time in the history of chemistry and physics.
It also fixes the scale of atomic chemistry. The Bohr radius \(a_0\) sets the size of the hydrogen atom (and, roughly, all atoms) at the Ångström scale, and the Rydberg energy \(13.6\text{ eV}\) sets the scale of chemical bond energies and ionisation energies — both numbers that recur throughout the rest of the periodic-trends story built on this unit.
Hypotheses
Proof
Result
Reading. One quantisation rule (\(L=n\hbar\)) applied to a classical circular Coulomb orbit forces both the radius and the energy to jump in discrete steps indexed by the integer \(n\); larger \(n\) means a larger, less tightly bound orbit, with energy climbing toward \(0\) (ionisation) as \(n\to\infty\).
Scope. Exact for any single-electron atom or ion: H, He\(^+\), Li\(^{2+}\), and so on, with \(Z\) the nuclear charge. Not valid, even approximately without modification, for any atom with two or more electrons.
Corollaries & converses
- The energy difference between two levels, \(\Delta E = 13.6\,Z^2\left(\dfrac{1}{n_1^2}-\dfrac{1}{n_2^2}\right)\text{ eV}\), combined with \(\Delta E=hc/\lambda\), is exactly the empirical Rydberg formula for the hydrogen line spectrum — the theorem this unit's next result (the Rydberg formula) makes explicit and general.
- The ionisation energy of hydrogen from its ground state is \(-E_1=13.6\,\text{eV}\), the reference value against which every other atom's first ionisation energy in this unit's periodic-trends result is measured.
- Converse fails: matching the correct energy levels does not mean the underlying orbital picture is correct. The full quantum-mechanical treatment (Schrödinger equation) reproduces exactly the same \(E_n=-13.6Z^2/n^2\,\text{eV}\) formula while rejecting the circular-orbit picture entirely — see Discussion.
Fails without
- Drop the one-electron restriction: for helium (\(Z=2\), two electrons), the same derivation cannot be run, because Step 1 assumed a single electron feels only the nuclear Coulomb force; with a second electron present, the potential energy term must include an electron–electron repulsion \(e^2/4\pi\varepsilon_0r_{12}\) that depends on both electrons' instantaneous separation, and the two-body circular-orbit ansatz no longer solves the resulting coupled problem in closed form.
- Drop the quantisation postulate (classical electrodynamics only): an accelerating charge radiates energy (Larmor's formula); a classical electron in a circular orbit continuously loses energy and its radius shrinks smoothly, predicting the atom collapses in about \(1.6\times10^{-11}\,\)s — an atom that cannot exist for more than a fraction of a nanosecond, in flat contradiction with observed matter. Quantisation of \(L\) is precisely what forbids all but a discrete set of radii, blocking the classical collapse.
Common errors
- Forgetting the factor of \(Z^2\) in the energy formula (and \(1/Z\) in the radius formula) when applying the result to a hydrogen-like ion rather than to hydrogen itself — He\(^+\) has \(E_1=-13.6\times4=-54.4\,\text{eV}\), not \(-13.6\,\text{eV}\).
- Treating the Bohr model as giving the correct orbital angular momentum of the electron. It does not: the true ground state has \(L=0\), while the Bohr model insists \(L=n\hbar\ge\hbar\) for every state, including \(n=1\).
- Applying the model, even qualitatively, to multi-electron atoms to "explain" periodic trends directly — the model has no term for electron–electron repulsion or shielding, both essential to real periodic trends (see this unit's periodic-trends result, which uses effective nuclear charge instead).
Discussion
Niels Bohr proposed this model in 1913, three years after Rutherford's gold-foil experiment established the nuclear atom and eleven years before de Broglie's matter-wave hypothesis and thirteen years before Schrödinger's equation. Bohr's genius move was to accept the classical planetary picture at face value but bolt on a single quantisation rule borrowed from Planck's 1900 treatment of blackbody radiation, and show that this one rule reproduces the Rydberg formula — an empirical fit that had stood, unexplained, for 25 years.
The model was superseded within about a decade by full quantum mechanics, and its central image — the electron as a tiny planet on a fixed circular track — is not how electrons actually behave; there are no orbits, only probability-density orbitals (the subject of this unit's quantum-numbers-and-orbitals result). Yet the energy-level formula \(E_n=-13.6Z^2/n^2\,\text{eV}\) survives completely unchanged when the correct calculation is redone with the Schrödinger equation for the hydrogen atom — a striking case of a model reaching the right quantitative answer through an incorrect physical mechanism, because for hydrogen specifically, the accidental degeneracy of the Coulomb potential collapses the true energy dependence (on both \(n\) and the orbital quantum number \(l\)) down to a dependence on \(n\) alone.
The deeper reason the Bohr formula survives is the Coulomb potential's special "accidental" \(SO(4)\) symmetry (beyond the ordinary \(SO(3)\) rotational symmetry every central potential has), first explained via the Laplace–Runge–Lenz vector; it is this extra symmetry that forces every orbital with the same principal quantum number \(n\) (regardless of \(l\)) to share exactly the same energy, which is exactly the single-index dependence \(E_n\) that Bohr's cruder model happened to stumble onto.
Common misconception: that the Bohr model is simply "an approximation" to the true quantum picture, in the sense of being close-but-imprecise. It is not an approximation in that sense at all — its energies are exact for hydrogen — but its physical picture (electrons on fixed circular tracks) is qualitatively wrong, not merely imprecise; it predicts a definite orbital radius and momentum simultaneously, which the uncertainty principle (a later, unit-CU-101 companion topic) forbids outright.
Worked examples
Reading. A single input rule (\(L=n\hbar\)) reproduces a measured spectral line to high precision, which is exactly why the model was accepted immediately in 1913 despite its later-discovered conceptual problems.
Scope. The same calculation, with the appropriate \(n_1,n_2\), gives every line of the hydrogen Balmer, Lyman, Paschen and higher series — the full content of the Rydberg formula, this unit's next result.
Problems
- Compute the ionisation energy of Li\(^{2+}\) (\(Z=3\)) from its ground state, and its ground-state orbital radius.
Solution
\(E_1=-13.6\times3^2=-122.4\,\text{eV}\), so the ionisation energy (energy required to remove the electron to \(r=\infty\), \(E=0\)) is \(+122.4\,\text{eV}\). The radius is \(r_1=a_0/3\approx0.176\,\text{Å}\) — smaller and more tightly bound than hydrogen or He\(^+\), continuing the \(Z^2\)/\(1/Z\) pattern of Worked Example 2. - Find the radius and speed of the electron in the \(n=4\) orbit of hydrogen, and check that the orbit's classical period is consistent with a bound (not escaping) electron.
Solution
\(r_4=4^2a_0=16a_0\approx8.46\,\text{Å}\). From Step 2, \(v=n\hbar/(m_er)\); substituting \(r_4\) and \(n=4\) gives \(v_4=\hbar/(4m_ea_0)=v_1/4\), where \(v_1=\alpha c\approx2.19\times10^6\,\text{m/s}\) is the \(n=1\) speed (a standard reference value), so \(v_4\approx5.5\times10^5\,\text{m/s}\). The orbital period \(T=2\pi r_4/v_4\) is finite and the energy \(E_4=-13.6/16=-0.85\,\text{eV}\) is negative, confirming a bound (non-escaping) orbit as expected for any finite \(n\). - A student calculates the Bohr-model energy levels for a neutral helium atom by simply setting \(Z=2\) in \(E_n=-13.6Z^2/n^2\,\text{eV}\) and comparing to the measured helium ionisation energy (\(24.6\,\text{eV}\)). Explain why this comparison is invalid, using the Hypotheses above.
Solution
Neutral helium has two electrons, not one, so the one-electron hypothesis is violated outright; the formula \(E_n=-13.6Z^2/n^2\) was derived (Step 1) assuming a single electron feels only the nuclear Coulomb attraction, with no electron–electron repulsion term. Plugging \(Z=2\) gives \(E_1=-54.4\,\text{eV}\) per electron, which is the correct energy for the hydrogen-like ion He\(^+\) (Worked Example 2) — not for neutral He, where electron–electron repulsion raises the actual first-ionisation energy to \(24.6\,\text{eV}\), roughly half the naive prediction. This is exactly the shielding effect explored properly in this unit's periodic-trends result. - Show that as \(n\to\infty\), \(E_n\to0^-\) and interpret this physically.
Solution
From the Result, \(E_n=-13.6Z^2/n^2\,\text{eV}\); as \(n\to\infty\), \(1/n^2\to0\), so \(E_n\to0\) from below (always negative for finite \(n\), approaching but never reaching zero). Physically, \(E=0\) is the threshold at which the electron is no longer bound to the nucleus (zero binding energy, infinite orbital radius, from \(r_n=n^2a_0/Z\to\infty\)); the levels \(E_n\) accumulate ever more densely just below this ionisation threshold, which is exactly what is observed spectroscopically as the Lyman/Balmer/etc. series limits, where the discrete lines converge to a continuum edge.